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Geometry of the string equations

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Abstract

The string equations of hermitian and unitary matrix models of 2D gravity are flatness conditions. These flatness conditions may be interpreted as the consistency conditions for isomonodromic deformation of an equation with an irregular singularity. In particular, the partition function of the matrix model is shown to be the tau function for isomonodromic deformation. The physical parameters defining the string equation are interpreted as moduli of meromorphic gauge fields, and the compatibility conditions can be interpreted as defining a “quantum” analog of a Riemann surface. In the latter interpretation, the equations may be viewed as compatibility conditions for transport on “quantum moduli space” of correlation functions in a theory of free fermions. We discuss how the free fermion field theory may be deduced directly from the matrix model integral. As an application of our formalism we discuss some properties of the BMP solutions of the string equations. We also mention briefly a possible connection to twistor theory.

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  1. Department of Physics, Yale University, 06511-8167, New Haven, CT, USA

    Gregory Moore

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Communicated by N. Yu. Reshetikhin

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Moore, G. Geometry of the string equations. Commun.Math. Phys. 133, 261–304 (1990). https://doi.org/10.1007/BF02097368

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